Elevation of Boiling Point

When a non-volatile solute is dissolved in a pure solvent, the boiling point of the resulting solution is always higher than that of the pure solvent. This phenomenon, known as boiling point elevation, is one of the four colligative properties of solutions — properties that depend solely on the number of solute particles present, not on their chemical identity. For example, dissolving table salt (\ceNaCl\ce{NaCl}) or sugar (\ceC12H22O11\ce{C_{12}H_{22}O_{11}}) in water both raise its boiling point, though by different amounts depending on the concentration and degree of dissociation. The physical explanation lies in vapour pressure. A pure solvent at its boiling point has a vapour pressure equal to atmospheric pressure. When a solute is dissolved, solute particles occupy positions at the liquid surface, reducing the number of solvent molecules that can escape into the gas phase. This lowers the vapour pressure of the solution (described by Raoult's Law). To restore the vapour pressure to atmospheric pressure — and thus reach the boiling point — a higher temperature is required. The elevation in boiling point is therefore a direct consequence of the solute-induced depression of vapour pressure. Boiling point elevation has important practical applications. It explains why antifreeze (ethylene glycol) raises the boiling point of engine coolant, why pasta water boils at a slightly higher temperature when salted, and why salt is used in industrial processes to achieve higher processing temperatures. The relationship between the magnitude of boiling point elevation and concentration is quantified by the ebullioscopic constant, KbK_b, a characteristic value for each solvent.

Key takeaways
  • Vapour Pressure and Raoult's Law
  • Why a Higher Temperature Is Needed
  • The Role of Molality
  • The van't Hoff Factor
  • The Ebullioscopic Constant KbK_b

Vapour Pressure and Raoult's Law

A liquid boils when its vapour pressure equals the external (atmospheric) pressure. For an ideal solution, Raoult's Law states that the vapour pressure of the solvent above the solution is Psolution=Xsolvent⋅Psolvent∗P_{solution} = X_{solvent} \cdot P^*_{solvent}, where XsolventX_{solvent} is the mole fraction of the solvent and Psolvent∗P^*_{solvent} is the vapour pressure of the pure solvent. Because Xsolvent<1X_{solvent} < 1 in any solution, Psolution<Psolvent∗P_{solution} < P^*_{solvent}: the vapour pressure is lowered.

Why a Higher Temperature Is Needed

Since the vapour pressure of the solution is lower than that of the pure solvent at the same temperature, the solution does not boil at the normal boiling point. The temperature must be raised until the vapour pressure of the solvent in the solution once again equals atmospheric pressure. This new, higher boiling point defines the elevation ΔTb\Delta T_b.

The Role of Molality

The boiling point elevation is proportional to the molality of solute particles (not the molarity). Molality mm is defined as moles of solute per kilogram of solvent: m=nsolutemsolvent(kg)m = \dfrac{n_{solute}}{m_{solvent(kg)}}. Molality is preferred over molarity because it is temperature-independent — it does not change as the solution expands or contracts with temperature fluctuations.

The van't Hoff Factor

For electrolytes that dissociate into ions, the effective number of particles is greater than the number of formula units dissolved. The van't Hoff factor ii accounts for this: i=1i = 1 for non-electrolytes, i=2i = 2 for fully dissociated 1:1 electrolytes like \ceNaCl\ce{NaCl} (which gives \ceNa+\ce{Na^+} and \ceCl−\ce{Cl^-}), and i=3i = 3 for \ceCaCl2\ce{CaCl_2} (giving \ceCa2+\ce{Ca^{2+}} and 2 \ceCl−2\,\ce{Cl^-}). The formula ΔTb=i⋅Kb⋅m\Delta T_b = i \cdot K_b \cdot m incorporates this factor.

The Ebullioscopic Constant KbK_b

The ebullioscopic constant KbK_b (from the Latin 'ebullire', to boil) is a solvent-specific constant with units of K ⋅ kg ⋅ mol−1\text{K}\,\cdot\,\text{kg}\,\cdot\,\text{mol}^{-1} (or equivalently °C ⋅ kg ⋅ mol−1°\text{C}\,\cdot\,\text{kg}\,\cdot\,\text{mol}^{-1}). For water, Kb=0.512 K ⋅ kg ⋅ mol−1K_b = 0.512\,\text{K}\,\cdot\,\text{kg}\,\cdot\,\text{mol}^{-1}. For benzene, Kb=2.53 K ⋅ kg ⋅ mol−1K_b = 2.53\,\text{K}\,\cdot\,\text{kg}\,\cdot\,\text{mol}^{-1}. It can be derived thermodynamically from the enthalpy of vaporisation: Kb=RTb2Msolvent1000 ΔHvapK_b = \dfrac{R T_b^2 M_{solvent}}{1000\,\Delta H_{vap}}, where TbT_b is the normal boiling point in Kelvin and MsolventM_{solvent} is the molar mass of the solvent in g/mol.

The Key Equation

ΔTb=i⋅Kb⋅m\Delta T_b = i \cdot K_b \cdot m
  • \Delta T_b — Boiling point elevation (K or °C): The increase in boiling point of the solution compared to the pure solvent. Always positive for a dissolved solute.
  • i — van't Hoff factor (dimensionless): The number of particles (ions or molecules) produced per formula unit of solute upon dissolution. i=1i=1 for glucose, i=2i=2 for \ceNaCl\ce{NaCl}, i=3i=3 for \ceCaCl2\ce{CaCl_2}.
  • K_b — Ebullioscopic constant (K·kg·mol⁻¹): A solvent-specific constant that reflects how strongly the solvent's boiling point responds to dissolved particles. For water: Kb=0.512 K ⋅ kg ⋅ mol−1K_b = 0.512\,\text{K}\,\cdot\,\text{kg}\,\cdot\,\text{mol}^{-1}.
  • m — Molality (mol·kg⁻¹): Moles of solute dissolved per kilogram of solvent. Not to be confused with molarity (mol per litre of solution).

Worked Example

Problem. A student dissolves 9.00 g of glucose (\ceC6H12O6\ce{C_6H_{12}O_6}, molar mass = 180.16 g/mol) in 250.0 g of water. What is the boiling point of this solution? (KbK_b for water = 0.512 K·kg·mol⁻¹; normal boiling point of water = 100.00 °C; glucose does not dissociate, so i=1i = 1.)

Tb=100.00 °C+0.10 °C=100.10 °CT_b = 100.00\,°\text{C} + 0.10\,°\text{C} = 100.10\,°\text{C}

Answer. The boiling point of the glucose solution is approximately 100.10 °C.

Figure
Diagram
Vapour Pressure vs. Temperature: Pure Solvent vs. SolutionTemperature (°C)Vapour PressureP_atmT_b (pure)T_b (solution)ΔT_bPure solventSolution
Origins · 1 minErnst Otto Beckmann and how this was discovered
EO
Ernst Otto Beckmann
1853–1923 · German

Ernst Otto Beckmann was a German chemist who made foundational contributions to the measurement of colligative properties. He invented the Beckmann thermometer — a highly sensitive, adjustable mercury thermometer capable of measuring temperature differences to 0.001 °C — which enabled precise determination of boiling point elevation and freezing point depression. His apparatus allowed chemists to determine molar masses of unknown compounds by measuring ΔT_b or ΔT_f, a technique that was central to chemistry for decades. Beckmann is also famous for discovering the Beckmann rearrangement (1886), a reaction in which a ketoxime is converted to an amide under acidic conditions — a completely unrelated but equally important contribution to organic chemistry.

  • Depression of Freezing Point — Freezing point depression is a closely parallel colligative property; both use the same molality-based formula structure with a cryoscopic constant (K_f) instead of K_b, making the two concepts natural companions.
  • Raoult's Law and Vapour Pressure Lowering — Boiling point elevation is mechanistically caused by vapour pressure lowering described by Raoult's Law. Understanding the vapour pressure relationship is essential to explaining why the boiling point rises.
  • Osmotic Pressure — Osmotic pressure is another colligative property that depends on the concentration of solute particles, illustrating the broader principle that solute presence affects multiple physical properties of solutions.
  • Molality and Solution Concentration — Molality is the specific concentration unit used in all colligative property calculations, and a solid understanding of how to calculate it is a prerequisite for applying the boiling point elevation formula correctly.
  • van't Hoff Factor and Electrolyte Dissociation — The van't Hoff factor i modifies the boiling point elevation formula for ionic compounds. Understanding ionic dissociation of electrolytes like NaCl and CaCl₂ is critical to accurately calculating ΔT_b for real solutions.